. "Advanced space plasma physics"@en . . "10" . "LEARNING OUTCOMES\nAfter completing this course, you are intended to have the ability to:\n\nnavigate the terminology and idiosyncrasies of space physics publications, enabling you\nto independently study and learn from research papers in the field\nderive different mathematical approaches to plasma physics from first principles, most\nimportantly: single-particle, kinetic and magnetohydrodynamic equations\ndiscern which of these approaches are applicable and practical for a given physical\nproblem\nobtain satellite measurement data from public data sources and interpret their results\nanalyze plasma wave properties for remote sensing of plasma conditions\nidentify and appraise plasma phenomena at the Sun, in the solar wind, in Earth's\nmagnetosphere and in the ionosphere\nindependently approach and study new plasma physics problems, and communicate\nyour findings\nCONTENT\nThese lectures are intended to advanced undergraduate and post-graduate students interested in space physics, plasma physics, applications of electrodynamics, statistical physics, hydrodynamics, etc. The course starts with plasma fundamentals, reviewing the basic concepts and looks more in depth to plasma distribution functions. The other topics include\n\nA detailed description of charged particle motion in electromagnetic fields, including time and spatially varying fields, including adiabatic invariants, motion in current sheets, and galactic cosmic rays will be covered.\nThe wave propagation in dielectric media, the main focus being on propagation through the layered ionosphere, but cold plasma wave theory will be briefly revised.\nA detailed coverage of the Vlasov theory and Landau damping\nA brief revision of magnetohydrodynamic (MHD) theory, the main focus will be put on subjects like force-free fields, flux ropes in space plasmas and magnetic helicity.\nPlasma Instabilities (micro- and macroinstabilities)\nTheory of collisionless shocks waves, dissipation of shocks, shock acceleration and solar energetic particles\nMagnetic reconnection (both theory and observations in space plasmas)\nBasics of solar dynamo\nRadiation and scattering (e.g., Bremsstrahlung, cyclotron and synchrotron)\nTransport (Fokker-Planck theory)\nThe contents of the course are oriented around the research fields that are investigated in the Space Physics research group. The course stays close to the possible thesis topics and concepts that actual research work in the field is based on." . . "Presential"@en . "FALSE" . . "Plasma Physics"@en . . . . . . . . . . . . . . . . . . . "Master's programme in Particle Physics and Astrophysical Sciences"@en . . "https://www.helsinki.fi/en/degree-programmes/particle-physics-and-astrophysical-sciences-masters-programme" . "120"^^ . "Presential"@en . "What are the laws of nature governing the universe from elementary particles to the development of the solar system, stars, and galaxies? In the Master’s Programme in Particle Physics and Astrophysical Sciences, you will focus on gaining a quantitative understanding of these phenomena.\n\nWith the expertise in basic research that you will gain in the programme, you might pursue a career in research. You will also acquire proficiency in the use of mathematical methods, IT tools and/or experimental equipment, as well as strong problem-solving and logical deduction skills. These will qualify you for a wide range of positions in the private sector.\n\nAfter completing the programme, you will:\n\n-Have wide-ranging knowledge of particle physical and/or astrophysical phenomena.\n-Have good analytical and computational skills and the ability to make sophisticated deductions.\n-Be able to apply theoretical, computational and/or experimental methods to the analysis and understanding of various phenomena.\n-Be able to apply your knowledge of particle physical and astrophysical phenomena as well as identify their interconnections.\n-Be able to formulate hypotheses and test them based your knowledge"@en . . . . "2"@en . "FALSE" . . . "Master"@en . "Thesis" . "no tuition, other costs may apply" . "Euro"@en . "15000.00" . "None" . "A Master’s degree in elementary particle physics or astrophysical sciences provides you with excellent qualifications for postgraduate education in research or for a career in diverse positions both in Finland and abroad. As a Master’s graduate you could begin a career in research and development in industry as well as in universities and other research institutes that enable you to conduct independent research on a topic that interests you."@en . "2"^^ . "TRUE" . "Upstream"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .